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XMM-Newton Observations of MBM 12: More Constraints on the Solar Wind Charge ...
International audience -
Statistical analysis of decay process upstream of the terrestrial bow shock
Thèse en Co-tutelle Université d'Orléans / Université Charles Pragues -
Solar wind pressure effects on Jupiter decametric radio emissions independent...
International audience -
Ion velocity distribution at the termination shock: 1-D PIC simulation
International audience -
Evidence of ion foreshock in 2-D PIC simulations of a curved collisionless sh...
International audience -
Solar wind charge exchange and local hot bubble X-ray emission with the DXL s...
International audience -
Update on modeling and data analysis of heliospheric solar wind charge exchan...
International audience -
Prototyping a global soft X-ray imaging instrument for heliophysics, planetar...
International audience -
High frequency turbulence in the solar wind : Hall magnetohydrodynamic model ...
Three-dimensional turbulence is characterized by its capacity to transfer energy from large to small scales where it is finally dissipated. When it occurs in a... -
Observation et modélisation de l'érosion des nuages magnétiques solaires par ...
Magnetic clouds (MCs), described as large-scale structures with a magnetic flux-rope topology, interact with the surrounding interplanetary medium during their... -
Solar Activity, Solar Wind and Geomagnetic Signatures
International audience -
Variation of Proton Flux Profiles with the Observer's Latitude in Simulated G...
We studied the variation of the shape of the proton intensity-time profiles in simulated gradual Solar Energetic Particle (SEP) events with the relative observer's... -
Geomagnetism during solar cycle 23: Characteristics
International audience -
Observations of the Interplanetary Hydrogen during Solar Cycles 23 and 24. Wh...
International audience
